1.Previous
3.Next

They examined a 10 MHz bandwidth with 52 kHz resolution and a 625 kHz bandwidth with 4 kHz resolution. The spectrometer was centered on the 21 cm hydrogen line in the rest frame of each observed star.

See also

* Ozma problem

References

Further reading

* Drake, F. D. "Project Ozma," Physics Today, 14, 140 (1961).
* Drake, Frank, "Project Ozma: The Search for

1.Previous
3.Next